We select galaxies from the IllustrisTNG hydrodynamical simulations (at 0≤ z≤ 2) and
characterize the shapes and evolutions of their UVJ and star formation rate–stellar mass …

The final product of galaxy evolution through cosmic time is the population of galaxies in the
local universe. These galaxies are also those that can be studied in most detail, thus …

The relation between galaxy stellar mass and gas-phase metallicity is a sensitive diagnostic
of the main processes that drive galaxy evolution, namely cosmological gas inflow, metal …

We use the chemical evolution predictions of cosmological hydrodynamic simulations with
our latest theoretical stellar population synthesis, photoionization, and shock models to …

We conduct a comprehensive analysis of the relationship between central galaxies and their
host dark matter halos, as characterized by the stellar mass–halo mass (SM–HM) relation …

We present an analysis of the host properties of 85 224 emission-line galaxies selected from
the Sloan Digital Sky Survey. We show that Seyferts and low-ionization narrow emission-line …

Aims. We study the relationship between the local environment of galaxies and their star
formation rate (SFR) in the Great Observatories Origins Deep Survey, GOODS, at. Methods …

We investigate the effect of metallicity calibrations, AGN classification, and aperture covering
fraction on the local mass-metallicity (MZ) relation using 27,730 star-forming galaxies from …

We examine the mass–metallicity relation for z≲ 1.6. The mass–metallicity relation follows a
steep slope with a turnover, or" knee," at stellar masses around 10 10 M☉. At stellar masses …

We present intermediate-resolution optical spectrophotometry of 65 galaxies obtained in
support of the Spitzer Infrared Nearby Galaxies Survey (SINGS). For each galaxy we obtain …